The past, present and future of observations of externally irradiated disks

Recent years have seen a surge of interest in the community studying the effect of ultraviolet radiation environment, predominantly set by OB stars, on protoplanetary disc evolution and planet formation. This is important because a significant fraction of planetary systems, potentially including our own, formed in close proximity to OB stars. This is a rapidly developing field, with a broad range of observations across many regions recently obtained or recently scheduled. In this paper, stimulated by a series of workshops on the topic, we take stock of the current and upcoming observations. We discuss how the community can build on this recent success with future observations to make progress in answering the big questions of the field, with the broad goal of disentangling how external photoevaporation contributes to shaping the observed (exo)planet population. Both existing and future instruments offer numerous opportunities to make progress towards this goal.

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Publication Details

Journal
The Open Journal of Astrophysics
Published
2025-05-02
DOI
https://doi.org/10.33232/001c.137538
Citations
7
Primary Topic
Astrophysical Phenomena and Observations
Type
article
Field-Weighted Citation Impact
8.08

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article

The past, present and future of observations of externally irradiated disks

Mari-Liis Aru, Jan Forbrich, S. Vicente, Raphaël Meshaka et al.
7 citations
The Open Journal of Astrophysics
Astrophysical Phenomena and Observations
8.08
article

The past, present and future of observations of externally irradiated disks

Mari-Liis Aru, Jan Forbrich, S. Vicente, Raphaël Meshaka, K. Gkimisi, Sierk van Terwisga, Jinyoung Serena Kim, M. G. Guarcello, Morten Andersen, Karina Maucó, Megan Reiter, Catherine Walsh, Peter Zeidler, M. C. Ramírez-Tannus, Saumya Gupta, Michael A. Kuhn, Nicholas P. Ballering, Javiera K. Díaz-Berríos, Giovanni Rosotti, Andrew J. Winter, Ilane Schroetter, W. J. Henney, R. J. Parker, James E. Owen, Paola Pinilla, Luke Keyte, Olivier Berné, Andrew D. Sellek, Ryan D. Boyden, Scott Paine, Megan J. Peatt, Arjan Bik, Lin Qiao, Megan Allen, L. Testi, S. Ramsay, N. J. Wright, G. Beccari, Gavin A. L. Coleman, Dominika Itrich, Giulia Ballabio, Thomas J. Haworth, C. F. Manara, Ciarán Rogers, Javier Goicoechea, Samuel Millstone, Joseph W. Eatson, Andrea Isella, Franck Le Petit, Jenny Frediani, Rossella Anania, Ling Luo, Tyger Peake
article en
7 citations

Abstract

Recent years have seen a surge of interest in the community studying the effect of ultraviolet radiation environment, predominantly set by OB stars, on protoplanetary disc evolution and planet formation. This is important because a significant fraction of planetary systems, potentially including our own, formed in close proximity to OB stars. This is a rapidly developing field, with a broad range of observations across many regions recently obtained or recently scheduled. In this paper, stimulated by a series of workshops on the topic, we take stock of the current and upcoming observations. We discuss how the community can build on this recent success with future observations to make progress in answering the big questions of the field, with the broad goal of disentangling how external photoevaporation contributes to shaping the observed (exo)planet population. Both existing and future instruments offer numerous opportunities to make progress towards this goal.

The Open Journal of AstrophysicsVol. 8
Space Telescope Science Institute (US), Space Science Institute (US), University of Leeds (GB), University of Arizona (US), University of Hertfordshire (GB), University of Lisbon (PT), Johns Hopkins University (US), Stockholm University (SE), Queen Mary University of London (GB), Université Fédérale de Toulouse Midi-Pyrénées (FR), University of Milan (IT), Université Paris-Saclay (FR), Observatoire de Paris (FR), Space Research Institute (AT), Instituto de Física Fundamental (ES), Max Planck Institute for Astronomy (DE), Observatoire de la Côte d’Azur (FR), Osservatorio Astronomico di Palermo (IT), Leiden Observatory, University College London (GB), Imperial College London (GB), University of Virginia (US), Keele University (GB), Rice University (US), Universidad Nacional Autónoma de México (MX), University of Sheffield (GB), University of Bologna (IT)
UK Research and Innovation, HORIZON EUROPE Framework Programme
Openalex Percentile: Top 3%
Astrophysical Phenomena and Observations
8.08
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